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Rho1 Cephei

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(Redirected from 28 Cephei) Star in the constellation Cepheus For other stars with this Bayer designation, see ρ Cephei.
Rho Cephei
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cepheus
Right ascension 22 26 42.40624
Declination +78° 47′ 09.0725″
Apparent magnitude (V) 5.84
Characteristics
Spectral type A2m
B−V color index −0.16
Astrometry
Proper motion (μ) RA: −13.33 mas/yr
Dec.: −36.95 mas/yr
Parallax (π)15.83 ± 0.23 mas
Distance206 ± 3 ly
(63.2 ± 0.9 pc)
Details
ρ Cep A
Mass2.00 M
Rotational velocity (v sin i)81 km/s
Age320 Myr
ρ Cep B
Mass0.51 M
Other designations
ρ Cep, 28 Cep, BD+78° 796, HD 213403, HIP 110787, HR 8578, SAO 10375, WDS J22267+7847AB
Database references
SIMBADdata

Rho Cephei (ρ Cephei) is a double star located in the northern constellation of Cepheus. As of 2014, the pair had an angular separation of 0.29 arc seconds along a position angle of 211.1°. This corresponds to a projected separation of 18.1 AU. Rho Cephei is faintly visible to the naked eye with an apparent visual magnitude of 5.84, and it forms an optical pair with the brighter star Rho Cephei. Based upon an annual parallax shift of 15.83 mas as seen from the Earth, Rho Cephei is located about 206 light years from the Sun.

The primary component is a chemically peculiar Am star with a stellar classification of A2m. It has twice the mass of the Sun and is around 320 million years old. The smaller companion may be the source of the X-ray emission from this location, as stars similar to the primary component do not generally produce detectable levels of X-rays.

References

  1. ^ van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  2. ^ Oja, T. (August 1991), "UBV photometry of stars whose positions are accurately known. VI", Astronomy and Astrophysics Supplement Series, 89 (2): 415–419, Bibcode:1991A&AS...89..415O.
  3. ^ De Rosa, R. J.; et al. (2013), "The VAST Survey - III. The multiplicity of A-type stars within 75 pc", Monthly Notices of the Royal Astronomical Society, 437 (2): 1216, arXiv:1311.7141, Bibcode:2014MNRAS.437.1216D, doi:10.1093/mnras/stt1932, S2CID 88503488.
  4. Royer, F.; et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i", Astronomy and Astrophysics, 393: 897–911, arXiv:astro-ph/0205255, Bibcode:2002A&A...393..897R, doi:10.1051/0004-6361:20020943, S2CID 14070763.
  5. "rho01 Cep". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-05-05.{{cite web}}: CS1 maint: postscript (link)
  6. De Rosa, R. J.; et al. (July 2011), "The Volume-limited A-Star (VAST) survey - I. Companions and the unexpected X-ray detection of B6-A7 stars", Monthly Notices of the Royal Astronomical Society, 415 (1): 854–866, arXiv:1103.4363, Bibcode:2011MNRAS.415..854D, doi:10.1111/j.1365-2966.2011.18765.x, S2CID 84181878.
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